New near-infrared CCD spectra of two infrared-excess B(e) stars

Details New near-infrared CCD spectra of two infrared-excess B(e) stars New near-infrared CCD spectra of two infrared-excess B(e) stars

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.254..413j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 254, Feb. 1, 1992, p. 413-418. Research supported by Co

Astronomy and Astrophysics

Astronomy

13

B Stars, Infrared Spectra, Infrared Stars, Near Infrared Radiation, Stellar Spectra, Charge Coupled Devices, Emission Spectra, H Alpha Line, Spectral Resolution, Ultraviolet Spectra

Scientific paper

Recent observations, mainly in the region from 0.7 to 1.03 micron, of two peculiar emission-line objects, HD 50138 and 45677, are reported, and the similarities and dissimilarities in their spectra are discussed. IR magnitudes showing the similarity of the flux distribution in the two stars as a function of the logarithm of the wavelength in the range 1 to 100 microns are illustrated. HD 50138 is classified as a transition object between a Be and a B(e) star.

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